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B. D. Simmons, C. M. Urry (Yale U.), S. Ravindranath (STScI), F. Bauer (Penn State U.), C. Conselice (Caltech), E. Chatzichristou (Yale U.), N. Grogin, A. M. Koekemoer, E. Schreier, R. Fosbury (ST-ECF), GOODS Team
There is growing evidence that the formation of galaxies and the growth of central black holes must be closely related. This ``grand unification'' of AGN and galaxies can be tested through studies of the AGN host galaxies. Using the deep multi-color HST ACS imaging data, we describe the morphologies of AGN host galaxies in the GOODS (Great Observatories Origins Deep Survey) southern field, which coincides with the Chandra Deep Field - South. We compare these to the morphologies of normal galaxies at the same (photometric) redshifts, also taken from the GOODS ACS data.
Ground-based imaging data were taken at ESO 2.2m, NTT, VLT, and NOAO 4m telescopes and made publicly available.
This work is supported by NASA.
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Bulletin of the American Astronomical Society, 34, #4
© 2002. The American Astronomical Soceity.